“…Conversely, a complex reduction profile was obtained for nZVI (Figure 5). The profile was split into three individual peaks centered at around 325 C, 530 C, and 730 C, that can be related to the H 2 consumption corresponding to the stepwise reduction of iron oxides, typically γ-Fe 2 O 3 (maghemite), Fe 3 O 4 (magnetite), and FeO (wüstite), respectively, to yield Fe 0 (metallic iron) (Ryu et al, 2008;Bychko, 2012). Since the intensity of each reduction peak is significantly different, it can be inferred the presence of mainly magnetite with wüstite to a lesser extent and a small amount of maghemite all of which, according to the TEM micrographs, would be located on the external surface of nZVI.…”